17-KEV NEUTRINO, SOLAR-NEUTRINO PUZZLE, AND SUPERNOVA 1987A

被引：8

作者：

CLINE, JM

机构：

[1] Department of Physics, McGill University, Montreal, Que. H3A 2T8

来源：

PHYSICAL REVIEW D | 1992年 / 45卷 / 05期

关键词：

D O I：

10.1103/PhysRevD.45.1628

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a model of the 17-keV neutrino which naturally admits Mikheyev-Smirnov-Wolfenstein oscillations of nu(e) and nu(mu) in the Sun, while avoiding forbidden nu(tau)-nu(tau)BAR oscillations. Alternatively, the large mixing angle needed for vacuum oscillations to reduce the solar nu(e) flux can be explained, in which case the nu(e) mass might naturally be close to its laboratory limit. The model is consistent with all known laboratory, cosmological, and astrophysical constraints, including the supernova bound on Dirac neutrino masses.

引用

页码：1628 / 1635

页数：8

共 42 条

[1] SOLAR-NEUTRINO PROBLEM - SOME OLD SOLUTIONS REEXAMINED [J].